Thermodynamics in the vicinity of a relativistic quantum critical point in 2+1 dimensions

preprint2013arXivOpen access

Abstract

We study the thermodynamics of the relativistic quantum O(NN) model in two space dimensions. In the vicinity of the zero-temperature quantum critical point (QCP), the pressure can be written in the scaling form $P(T)=P(0)+N(T^3/c^2)\calF_N(Δ/T)$ where cc is the velocity of the excitations at the QCP and ΔΔ is a characteristic zero-temperature energy scale. Using both a large-NN approach to leading order and the nonperturbative renormalization group, we compute the universal scaling function $\calF_N$. For small values of NN (N≲10N\lesssim 10) we find that $\calF_N(x)$ is nonmonotonous in the quantum critical regime (∣x∣≲1|x|\lesssim 1) with a maximum near x=0x=0. The large-NN approach -- if properly interpreted -- is a good approximation both in the renormalized classical (x≲−1x\lesssim -1) and quantum disordered (x≳1x\gtrsim 1) regimes, but fails to describe the nonmonotonous behavior of $\calF_N$ in the quantum critical regime. We discuss the renormalization-group flows in the various regimes near the QCP and make the connection with the quantum nonlinear sigma model in the renormalized classical regime. We compute the Berezinskii-Kosterlitz-Thouless transition temperature in the quantum O(2) model and find that in the vicinity of the QCP the universal ratio $\Tkt/ρ_s(0)$ is very close to π/2π/2, implying that the stiffness $ρ_s(\Tkt^-)$ at the transition is only slightly reduced with respect to the zero-temperature stiffness ρs(0)ρ_s(0). Finally, we briefly discuss the experimental determination of the universal function $\calF_2$ from the pressure of a Bose gas in an optical lattice near the superfluid--Mott-insulator transition.

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